Search: onr:"swepub:oai:DiVA.org:uu-487249" > The Long-Term Evolu...
Fältnamn | Indikatorer | Metadata |
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000 | 05118naa a2200529 4500 | |
001 | oai:DiVA.org:uu-487249 | |
003 | SwePub | |
008 | 221103s2022 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4872492 URI |
024 | 7 | a https://doi.org/10.1007/s11214-022-00924-02 DOI |
040 | a (SwePub)uu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a for2 swepub-publicationtype |
100 | 1 | a Gillmann, Cedricu Rice Univ, Dept Earth Environm & Planetary Sci, Houston, TX 77005 USA.4 aut |
245 | 1 0 | a The Long-Term Evolution of the Atmosphere of Venus :b Processes and Feedback Mechanisms Interior-Exterior Exchanges |
264 | c 2022-10-07 | |
264 | 1 | b Springer,c 2022 |
338 | a electronic2 rdacarrier | |
520 | a This work reviews the long-term evolution of the atmosphere of Venus, and modulation of its composition by interior/exterior cycling. The formation and evolution of Venus's atmosphere, leading to contemporary surface conditions, remain hotly debated topics, and involve questions that tie into many disciplines. We explore these various inter-related mechanisms which shaped the evolution of the atmosphere, starting with the volatile sources and sinks. Going from the deep interior to the top of the atmosphere, we describe volcanic outgassing, surface-atmosphere interactions, and atmosphere escape. Furthermore, we address more complex aspects of the history of Venus, including the role of Late Accretion impacts, how magnetic field generation is tied into long-term evolution, and the implications of geochemical and geodynamical feedback cycles for atmospheric evolution. We highlight plausible end-member evolutionary pathways that Venus could have followed, from accretion to its present-day state, based on modeling and observations. In a first scenario, the planet was desiccated by atmospheric escape during the magma ocean phase. In a second scenario, Venus could have harbored surface liquid water for long periods of time, until its temperate climate was destabilized and it entered a runaway greenhouse phase. In a third scenario, Venus's inefficient outgassing could have kept water inside the planet, where hydrogen was trapped in the core and the mantle was oxidized. We discuss existing evidence and future observations/missions required to refine our understanding of the planet's history and of the complex feedback cycles between the interior, surface, and atmosphere that have been operating in the past, present or future of Venus. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a Venus | |
653 | a Atmosphere | |
653 | a Coupled evolution | |
653 | a Feedback cycles | |
653 | a Volatile exchanges | |
700 | 1 | a Way, Michael J.u Uppsala universitet,Teoretisk astrofysik,NASA, Goddard Inst Space Studies, 2880 Broadway, New York, NY 10025 USA4 aut0 (Swepub:uu)micwa958 |
700 | 1 | a Avice, Guillaumeu Univ Paris Cite, CNRS, Inst Phys Globe Paris, F-75005 Paris, France.4 aut |
700 | 1 | a Breuer, Dorisu DLR, Inst Planetary Res, D-12489 Berlin, Germany.4 aut |
700 | 1 | a Golabek, Gregor J.u Univ Bayreuth, Bayer Geoinst, D-95440 Bayreuth, Germany.4 aut |
700 | 1 | a Hoening, Dennisu Potsdam Inst Climate Impact Res, Potsdam, Germany.;VU, Dept Earth Sci, Amsterdam, Netherlands.4 aut |
700 | 1 | a Krissansen-Totton, Joshuau Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA.4 aut |
700 | 1 | a Lammer, Helmutu Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut |
700 | 1 | a O'Rourke, Joseph G.u Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA.4 aut |
700 | 1 | a Persson, Moau Univ Paul Sabatier Toulouse III, CNRS, Inst Rech Astrophys & Planetol, Ctr Natl Etud Spatiales, Toulouse, France.4 aut |
700 | 1 | a Plesa, Ana-Catalinau DLR, Inst Planetary Res, D-12489 Berlin, Germany.4 aut |
700 | 1 | a Salvador, Arnaudu No Arizona Univ, Dept Astron & Planetary Sci, Box 6010, Flagstaff, AZ 86011 USA.;Univ Arizona, Habitabil Atmospheres & Biosignatures Lab, Tucson, AZ USA.;Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA.4 aut |
700 | 1 | a Scherf, Manuelu Austrian Acad Sci, Space Res Inst, Graz, Austria.;Karl Franzens Univ Graz, Inst Phys, Graz, Austria.;Tech Univ, Inst Geodesy, Graz, Austria.4 aut |
700 | 1 | a Zolotov, Mikhail Y.u Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA.4 aut |
710 | 2 | a Rice Univ, Dept Earth Environm & Planetary Sci, Houston, TX 77005 USA.b Teoretisk astrofysik4 org |
773 | 0 | t Space Science Reviewsd : Springerg 218:7q 218:7x 0038-6308x 1572-9672 |
856 | 4 | u https://doi.org/10.1007/s11214-022-00924-0y Fulltext |
856 | 4 | u https://uu.diva-portal.org/smash/get/diva2:1708210/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-487249 |
856 | 4 8 | u https://doi.org/10.1007/s11214-022-00924-0 |
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